It is hard to imagine that any astronomical phenomenon could escape our latest and most powerful telescopes, but an international research team has now forecast some of the exotic discoveries that will only be able to be studied with the forthcoming Square Kilometre Array (SKA).

The team, including Dr. Davide Burlon and Dr. Tara Murphy from the University of Sydney’s School of Physics, has calculated that the SKA will reveal the lingering footprints of tens of thousands of enigmatic cosmic explosions known as ‘gamma-ray bursts.’

Dr. Giancarlo Ghirlanda at the National Institute for Astrophysics in Italy led the team.

“With current telescopes, we see a bright gamma-ray burst somewhere in the universe around once per day, but new radio telescopes will soon be able to see an afterglow of the explosion after the initial burst has faded away,” explains Dr. Burlon, a postdoctoral researcher in the ARC Centre of Excellence for All-sky Astrophysics (CAASTRO).

“This afterglow can generally take weeks to gradually decay and teaches us incredible amounts about both the initial explosion and its neighborhood.”

The catch is that a gamma-ray burst is not an explosion that can be seen from all directions but is comprised of a very narrow, energetic jet. So an observer needs to be looking down the barrel of the jet at the right time otherwise it is invisible.

The radio afterglow should be visible from any direction however and for long periods of time, even if the burst is missed. These afterglows without a burst are known as orphan afterglows — they’re a phenomenon that astronomers have been looking for without success, until now.

“From the rate at which we detect gamma-ray bursts, we were able to predict that with the power of a sensitive new telescope like the SKA, orphan afterglows should be seen 700 times more often than their gamma-ray bursts.” says Dr. Burlon.

“The unprecedented sensitivity and wide field-of view of the SKA means that orphan afterglows should be visible for months or even years before eventually disappearing — bubbling across the sky more than ten thousand times per year.”

Of course, the SKA’s view of the sky will be full of all sorts of objects and events, such as supernova explosions and flaring black holes that are more common than orphan afterglows.

“In this new era of radio astronomy, one of the challenges will be to disentangle these different classes of radio sources.” says Dr. Tara Murphy, CAASTRO Associate Investigator and project leader of the “Variables and Slow Transients” survey with the Australian SKA Pathfinder (ASKAP).

The SKA will join the Australian SKA precursor telescope ASKAP and the South African SKA precursor MeerKAT in painting an entirely new picture of the ‘radio sky.’

“The SKA will not only allow us to finally see these orphan afterglows but help us understand how gamma-ray bursts produce such powerful, narrow jets and will cast new light on the big question of just what causes gamma-ray bursts in the first place,” concludes Dr. Ghirlanda.

PIO Contact:
Verity Leatherdale
University of Sydney
+61 (0)2) 9351 4312, +61 (0)4 0306 7342
verity.leatherdale@sydney.edu.au

Science Contacts:
Dr. Davide Burlon
University of Sydney
+61 (0)2 9114 2149
dburlon@physics.usyd.edu.au

Dr. Tara Murphy
University of Sydney
+61 (0)2 9351 3041
tara.murphy@sydney.edu.au

Dr. Wiebke Ebeling
Curtin University
+61 (0)8 9266 9174, +61 (0)4 2393 3444
wiebke.ebeling@curtin.edu.au

Reference:
“GRB Orphan Afterglows in Present and Future Radio Transient Surveys,” G. Ghirlanda, D. Burlon, G. Ghisellini, R. Salvaterra, M. G. Bernardini, S. Campana, S. Covino, P. D’Avanzo, V. D’Elia, A. Melandri, T. Murphy, L. Nava, S. D. Vergani, G. Tagliaferri, to appear in Publications of the Astronomical Society of Australia [preprint:
http://arxiv.org/abs/1402.6338].

The ARC Center of Excellence for All-sky Astrophysics (CAASTRO) is a collaboration between The University of Sydney, The Australian National University, The University of Melbourne, Swinburne University of Technology, The University of Queensland, The University of Western Australia and Curtin University, the latter two par
ticipating together as the International Centre for Radio Astronomy Research (ICRAR). CAASTRO is funded under the Australian Research Council (ARC) Center of Excellence program, with additional funding from the seven participating universities and from the NSW State Government’s Science Leveraging Fund.